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Chapter 11. Rotational Dynamics - Physics and Astronomy @ UGA · Chapter 11. Rotational Dynamics As...

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Chapter 11. Rotational Dynamics As we did for linear (or translational) motion, we studied kinematics (motion without regard to the cause) and then dynamics (motion with regard to the cause), we now proceed in a similar fashion We know that forces are responsible for linear motion We will now see that rotational motion is caused by torques Consider a wrench of length L=r
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Page 1: Chapter 11. Rotational Dynamics - Physics and Astronomy @ UGA · Chapter 11. Rotational Dynamics As we did for linear (or translational) motion, we studied kinematics (motion without

Chapter 11. Rotational Dynamics   As we did for linear (or translational) motion, we studied kinematics (motion without regard to the cause) and then dynamics (motion with regard to the cause), we now proceed in a similar fashion

  We know that forces are responsible for linear motion

  We will now see that rotational motion is caused by torques

  Consider a wrench of length L=r

Page 2: Chapter 11. Rotational Dynamics - Physics and Astronomy @ UGA · Chapter 11. Rotational Dynamics As we did for linear (or translational) motion, we studied kinematics (motion without

F

τ = rF

r

Torque

Units of N m

Not work or energy, do not use Joules

is called the lever arm. Must always be perpendicular to the force

If the force is not perpendicular to the level arm, we need to find the component that is perpendicular (either the force or the lever arm)

r

Page 3: Chapter 11. Rotational Dynamics - Physics and Astronomy @ UGA · Chapter 11. Rotational Dynamics As we did for linear (or translational) motion, we studied kinematics (motion without

φ

F F sinφ

τ = rF sinφ

If φ=0, then the torque is zero

r  Therefore, torques (force times length) are responsible for rotational motion

Page 4: Chapter 11. Rotational Dynamics - Physics and Astronomy @ UGA · Chapter 11. Rotational Dynamics As we did for linear (or translational) motion, we studied kinematics (motion without

Newton’s 2nd Law for Rotational Motion

F=Ft

r m

  The torque for a point-particle of mass m a distance r from the rotation axis is

τ = rFtFt = mat, at = rα⇒ τ = matr = mr2α

Axis of rotation

  Define I = mr2 = Moment of Inertia for a point particle; a scalar, units of kg m2

  A rigid body is composed of many, many particles

Page 5: Chapter 11. Rotational Dynamics - Physics and Astronomy @ UGA · Chapter 11. Rotational Dynamics As we did for linear (or translational) motion, we studied kinematics (motion without

of mass mi which are ri from the axis of rotation

  Each of these masses creates a torque about the axis of rotation

....

2222

2111

ατατrmrm

== m1

m2

r1

r2

Rotation axis

  Sum up all torques due to all particles

∑∑

∑ ∑

==

=

ατ

ατ

IrmIrm

ii

iii2

2 α  is the same for all particles

I =moment of inertia for the rigid body. It is different for different shaped objects and for different axes of rotation. Table 10.1.

Page 6: Chapter 11. Rotational Dynamics - Physics and Astronomy @ UGA · Chapter 11. Rotational Dynamics As we did for linear (or translational) motion, we studied kinematics (motion without

  For a thin rod of mass M and length L

L/2 L 2121 MLI =

231MLI =

  The last equation is Newton’s 2nd Law for rotation. Compare to the translational form

Example Problem

A rotating door is made of 4 rectangular panes each with a mass of 85 kg. A person pushes on the outer edge of one pane with a force of 68 N, directed perpendicular to the pane. Determine the door’s α.

amFI =⇔= ∑∑ ατ

Page 7: Chapter 11. Rotational Dynamics - Physics and Astronomy @ UGA · Chapter 11. Rotational Dynamics As we did for linear (or translational) motion, we studied kinematics (motion without

L

F IFLIFL

I

=⇒=

=∑αα

ατ

Given: L = 1.2 m, mpane=85 kg, F=68 N

From Table 10.1, moment of inertia for a thin rectangular rod is (same as a thin sheet)

Since there are 4 panes.

2342

31 MLIMLI doorpane =⇒=

2srad

m kgN

234

50.050.0)m 2.1)(kg 85(4

)N 68(343

====

==

MLF

MLFL

IFL

α

α

Page 8: Chapter 11. Rotational Dynamics - Physics and Astronomy @ UGA · Chapter 11. Rotational Dynamics As we did for linear (or translational) motion, we studied kinematics (motion without

Example Problem The parallel axis theorem provides a useful way to calculate I about an arbitrary axis. The theorem states that I = Icm + MD2, where Icm is the moment of inertia of an object (of mass M) with an axis that passes through the center of mass and is parallel to the axis of interest. D is the perpendicular distance between the two axes. Now, determine I of a solid cylinder of radius R for an axis that lies on the surface of the cylinder and perpendicular to the circular ends.

Solution: The center of mass of the cylinder is on a line defining the axis of the cylinder

Page 9: Chapter 11. Rotational Dynamics - Physics and Astronomy @ UGA · Chapter 11. Rotational Dynamics As we did for linear (or translational) motion, we studied kinematics (motion without

R

221 MRIcm =From Table 10.1:

From the parallel axis theorem with D=R:

Apply to thin rod:

cm

22322

212 MRMRMRMDII cm =+=+=

L/2 L 2121 MLIcm =

231

22

1212

2MLLMMLMDII cm =

+=+=

Page 10: Chapter 11. Rotational Dynamics - Physics and Astronomy @ UGA · Chapter 11. Rotational Dynamics As we did for linear (or translational) motion, we studied kinematics (motion without

Rotational Work

  For translational motion, we defined the work as

  For rotational motion

W = Fddθ

r

r s = arc length

= rθ

s

d

F d

W = Fdd = Ftrθ = (Ftr)θWR = τ θ

Ft

Units of N m or J when θ is in radians

Rotational Kinetic Energy   For translational motion, the K was defined

Page 11: Chapter 11. Rotational Dynamics - Physics and Astronomy @ UGA · Chapter 11. Rotational Dynamics As we did for linear (or translational) motion, we studied kinematics (motion without

22212

2121

)(,

ωωω

mrrmKrmK t

==== v since v2

  For a point particle I = mr2, therefore

  Or for a rigid body

  For a rigid body that has both translational and rotational motion, its total kinetic energy is

  The total mechanical energy is then

Krot = 12 Iω

2

Krot = 12 miri

2ω 2 = 12∑ Iω 2 = Krot

Ktotal = K + Krot = 12mv

2 + 12 Iω

2

Etotal = 12mv

2 + 12 Iω

2 + mgy + 12 kx

2

Page 12: Chapter 11. Rotational Dynamics - Physics and Astronomy @ UGA · Chapter 11. Rotational Dynamics As we did for linear (or translational) motion, we studied kinematics (motion without

Example A car is moving with a speed of 27.0 m/s. Each wheel has a radius of 0.300 m and a moment of inertia of 0.850 kg m2. The car has a total mass (including the wheels) of 1.20x103 kg. Find (a) the translational K of the entire car, (b) the total Krot of the four wheels, and (c) the total K of the car.

Solution:

Given: vcar = 27.0 m/s, mcar = 1.20x103 kg, rw = 0.300 m, Iw = 0.850 kg m2

Page 13: Chapter 11. Rotational Dynamics - Physics and Astronomy @ UGA · Chapter 11. Rotational Dynamics As we did for linear (or translational) motion, we studied kinematics (motion without

K = 12 mcarvcar

2 = 12 (1.2x103)(27.0)2

K = 4.37x105 J

Krot = 12 Iω

2 = 12 Iw

vt

rw

2

= 12 Iw

vcar

rw

2

Krot = 12 (0.850)(27.0 /0.300)2

= 3.44x103 JKwheels = 4Krot =1.38x104 JKtotal = K + Kwheels= 4.37x105 +1.38x104 = 4.51x105 J

a)

b)

c)

Page 14: Chapter 11. Rotational Dynamics - Physics and Astronomy @ UGA · Chapter 11. Rotational Dynamics As we did for linear (or translational) motion, we studied kinematics (motion without

Example Problem A tennis ball, starting from rest, rolls down a hill into a valley. At the top of the valley, the ball becomes airborne, leaving at an angle of 35° with respect to the horizontal. Treat the ball as a thin-walled spherical shell and determine the horizontal distance the ball travels after becoming airborne.

1.8 m θ

x

0

1 2

3

4

Page 15: Chapter 11. Rotational Dynamics - Physics and Astronomy @ UGA · Chapter 11. Rotational Dynamics As we did for linear (or translational) motion, we studied kinematics (motion without

Solution:

Given: v0 = 0, ω0 = 0, y0 = 1.8 m = h, y1 = y2 = y4 = 0, θ2 = 35°, x2 = 0, I=(2/3)MR2

Find: x4 ?

Method: As there is no “friction” or air resistance in the problem, therefore no non-conservative forces, we can use conservation of mechanical energy

1222

1222

12

212

1212

11

0

)0(v)0(vEmgImE

mgImEmghE

=++=++=

=

ωω

mgyImEtotal ++= 2212

21 v ω

Page 16: Chapter 11. Rotational Dynamics - Physics and Astronomy @ UGA · Chapter 11. Rotational Dynamics As we did for linear (or translational) motion, we studied kinematics (motion without

m/s 6.48)/56(9.80)(1.

5/6 v

vvv

)/v)((v

vvbut v ,v

Since ,v v

2

226

5223

1222

1

22

232

212

221

2

222

1222

1

210

2121

==

=⇒

=+=

+=

=

=+=

==

==⇒

gh

gh

rmrmmgh

rImmghEEE

t

t ωω

ωω

Velocity of ball equals tangential velocity at edge of ball

Now, use 2D kinematic equations for projectile motion

Page 17: Chapter 11. Rotational Dynamics - Physics and Astronomy @ UGA · Chapter 11. Rotational Dynamics As we did for linear (or translational) motion, we studied kinematics (motion without

m 0.25

35sin35cos)8.1(125

sincos12g

sincos25

6g

sincos2v/sinvcos2v/v2v

v)vv(/2vv2

vv0 ),(vv

vsinvvvcosvv

4

224

222222

4

2222224

4244221

24

2442

422

22424

4222

4222

=

==

==

===++=

=⇒−=−−=−

=−−=−==

==

x

hx

ghx

ggxttxxgtgt

gttttg

yx

xxx

yy

yy

yy

yy

xx

θθ

θθθθθθ

θθ

v2

v4

Page 18: Chapter 11. Rotational Dynamics - Physics and Astronomy @ UGA · Chapter 11. Rotational Dynamics As we did for linear (or translational) motion, we studied kinematics (motion without

Example Problem   A mass m1 (=15.0 kg) and a mass m2

(=10.0 kg) are suspended by a pulley that has a radius R (=10.0 cm) and a mass M (=3.00 kg). The cord has negligible mass and causes the pulley to rotate without slipping. The pulley rotates about its axis without friction. The masses start from rest at a distance h (=3.00 m) part. Treating the pulley as a uniform disk, determine the speeds of the two masses as they pass each other.


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